Pages that link to "Item:Q5350381"
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The following pages link to Black hole continuum spectra as a test of general relativity: quadratic gravity (Q5350381):
Displaying 10 items.
- Difficulties of quantitative tests of the Kerr-hypothesis with X-ray observations of mass accreting black holes (Q1622151) (← links)
- Thin accretion disk signatures of scalarized black holes in Einstein-scalar-Gauss-Bonnet gravity (Q2233899) (← links)
- Black hole based tests of general relativity (Q2807418) (← links)
- Can the slow-rotation approximation be used in electromagnetic observations of black holes? (Q2811460) (← links)
- Publisher’s Note: Kerr Black Holes Are Not Unique to General Relativity [Phys. Rev. Lett.<b>100</b>, 091101 (2008)] (Q3107899) (← links)
- The exact dynamical Chern–Simons metric for a spinning black hole possesses a fourth constant of motion: a dynamical-systems-based conjecture (Q3120868) (← links)
- In quest of axionic hairs in quasars (Q5022256) (← links)
- Testing black holes in non-linear electrodynamics from the observed quasi-periodic oscillations (Q5101142) (← links)
- Black hole shadow as a test of general relativity: quadratic gravity (Q5218335) (← links)
- A novel test of gravity via black hole eikonal correspondence (Q6055972) (← links)